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Ammonite zones of northern Chihuahua - New Mexico Geological ...

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98 NEW MEXICO GEOLOGICAL SOCIETY-TWENTIETH FIELD CONFERENCE<br />

W. T. Keller had a group <strong>of</strong> Swiss geologists in <strong>northern</strong><br />

<strong>Chihuahua</strong>, working for "El Aguila" (La Compania de<br />

Méxicana de Shell ). Keller collected Campanian fossils in<br />

the vicinity <strong>of</strong> Ojinaga and La Mula, and Jurassic fossils at<br />

San Sostenes. These fossils were taken to Tampico and were<br />

eventually deposited in the University <strong>of</strong> Texas collections<br />

as the "El Aguila" part <strong>of</strong> the W. S. Adkins collection.<br />

These fossils had also been seen by Burkhardt (1933) and<br />

still accompany a label bearing the name <strong>of</strong> the collector,<br />

the date, and the locality.<br />

REMARKS ON<br />

AMMONITE ZONATION<br />

The ammonite <strong>zones</strong> <strong>of</strong> Tables 1 and 2 are incomplete.<br />

There are three reasons for incomplete ammonite zonation:<br />

(1) collection failure, (2) wrong environment, e. g., ammonites<br />

are not found in non-marine rocks, nor are they<br />

found in rudistid-bearing strata, and ( 3) lacunae. The first<br />

two examples appear to be mainly responsible for the<br />

absence <strong>of</strong> many ammonite <strong>zones</strong> in <strong>northern</strong> <strong>Chihuahua</strong>.<br />

JURASSIC ZONES<br />

I have listed only two Jurassic <strong>zones</strong> from <strong>northern</strong> <strong>Chihuahua</strong>.<br />

W. S. Adkins and R. E. King collected the fossils,<br />

and Imlay (1943) described them. However, there may be<br />

more than two <strong>zones</strong>, as indicated by the age comparisons<br />

<strong>of</strong> Imlay (1943, p. 529) .<br />

The absence <strong>of</strong> Upper Kimmeridgian and Lower Tithonian<br />

<strong>zones</strong> in the Placer de Guadalupe area is probably<br />

the result <strong>of</strong> collection failure in rocks that do not abound<br />

with fossils. Upper Tithonian and Lower Neocomian<br />

(Berriasian and Valanginian <strong>zones</strong>) are likwise probably<br />

absent by collection failure in this vicinity; they could be<br />

cut out by complex structure, or these slightly fossiliferous<br />

beds may not as yet have yielded fossils. No one has found<br />

a Jurassic-Cretaceous unconformity in this area, but I must<br />

admit that not many have tried. Fossils <strong>of</strong> the Kossmatia<br />

rancheriaensis Imlay zone also occur in the Jurassic Malone<br />

Formation <strong>of</strong> the Malone Mountains; the specimen that I<br />

have identified is a Kossmatia kingi Imlay. Otherwise, the<br />

Jurassic is not known north or northeast <strong>of</strong> the vicinity <strong>of</strong><br />

Placer de Guadalupe, unless the Jurassic at Sierra de Ojo<br />

Caliente, stop 4 <strong>of</strong> trip A-13, 20th International <strong>Geological</strong><br />

Congress (Diaz, 1956, p. 312, Fig. 4) has been correctly<br />

dated.<br />

CRETACEOUS ZONES<br />

The collection in the summer <strong>of</strong> 1968 by D. S. Webb <strong>of</strong><br />

a good specimen <strong>of</strong> Leopoldia victoriensis Imlay (1938)<br />

from the sandstones along the highway south <strong>of</strong> Samalayuca<br />

has changed the age <strong>of</strong> these rocks, formerly reported as<br />

Jurassic by William E. Humphrey (Diaz, 1956, p. 28) on<br />

field identification only. These rocks are lower Hauterivian.<br />

The same rocks with the same fossils occur at Placer de<br />

Guadalupe where Bridges (1962, 1965, pp. 74-76) reported<br />

them as Jurassic because I made misidentifications similar<br />

to Humphrey's. An isolated specimen, in different lithology,<br />

<strong>of</strong> Leopoldia sp. cf. leopoldinus (d'Orbigny), collected by<br />

DeFord from near the picachos in the vicinity <strong>of</strong> Placer de<br />

Guadalupe, likewise is lower Hauterivian. Two Lower Cretaceous<br />

ammonites (presumably pre-Aptian) are rumored<br />

to have come from near Cuchillo Parado, but these seem to<br />

be misplaced. No pre-Aptian ammonites from <strong>northern</strong><br />

<strong>Chihuahua</strong>, other than those mentioned above, are known<br />

to the writer.<br />

Jurassic and Cretaceous fossils are reported at Sierra de<br />

Ojo Caliente (Diaz, 1956, p. 26, 31, 32 ). I have seen no<br />

identifiable fossils from this locality.<br />

The absence <strong>of</strong> upper Hauterivian, Barremian, and most<br />

<strong>of</strong> the Lower Aptian ammonites from <strong>northern</strong> <strong>Chihuahua</strong><br />

can usually be attributed to the occurrence <strong>of</strong> the wrong<br />

facies. In many localities the Navarette evaporite section is<br />

overlain by continental deposits, as on the west flank <strong>of</strong> the<br />

Sierra de la Aldea, east <strong>of</strong> Cuchillo Parado. At this locality,<br />

above the evaporites, pulmonate land snails have been collected<br />

by Young, Powell, Diaz, and DeFord. In the southern<br />

Quitman Mountains, dinosaur bones were collected by<br />

Donald Campbell (1968) and Bill Jones (1968) from the<br />

Las Vigas formation. How much <strong>of</strong> the Las Vigas Formation<br />

is terrestrial is debatable, but the Las Vigas and Navarette<br />

formations certainly represent environments inhospitable<br />

to ammonites.<br />

The first ammonites above the lower Hauterivian represent<br />

the latest Lower Aptian. These are Cheloniceras sp.,<br />

one specimen from the Sierra del Presidio; Cheloniceras<br />

adkinsi Scott, from the southern Quitman Mountains,<br />

which may not be a Cheloniceras; and a specimen <strong>of</strong> Cheloniceras<br />

from just above the redbed sequence on the east<br />

flank <strong>of</strong> Sierra Cuervo, north <strong>of</strong> Aldama. Only in these<br />

three areas have probable late Lower Aptian fossils been<br />

collected.<br />

Upper Aptian fossils are well known in <strong>northern</strong> <strong>Chihuahua</strong><br />

and adjacent Trans-Pecos Texas (Table 1).<br />

The zone <strong>of</strong> Dufrenoyia justinae (Hill) is not as widespread<br />

as heret<strong>of</strong>ore assumed, since myself and others have<br />

misidentified Hypacanthoplites bakeri Scott as D. justinae<br />

on more than one occasion. In addition, the Dufrenovia<br />

justinae zone may represent other <strong>zones</strong> too, but the geological<br />

sections have not been collected in detail, and none<br />

have received the type <strong>of</strong> study necessary to produce exact<br />

collections.<br />

Overlying the zone <strong>of</strong> Dufrenoyia justinae in the southern<br />

Quitman Mountains <strong>of</strong> Trans-Pecos Texas, the Sierra<br />

del Presidio, and the Bisbee district <strong>of</strong> southeastern Arizona<br />

is the zone <strong>of</strong> Kazanskyella trinitense (Scott). Finer collecting<br />

may also produce a more detailed zonation at this level.<br />

This fauna has not been collected to the south <strong>of</strong> these<br />

areas, probably because it is replaced by the late Aptianlower<br />

Albian rudistid complex. Gillerman (1958, pp. 47-50)<br />

collected a fauna <strong>of</strong> approximately the same age from the<br />

Carbonate Hill Limestone in the central Peloncillo Mountains.<br />

Some <strong>of</strong> his specimens seem to be closely related to<br />

Kazanskyella n. sp. from the Bexar Shale in the Spahn well<br />

in Gonzales County, south Texas. I also have a good specimen<br />

<strong>of</strong> Kazanskyella trinitense (Scott) from the Sierra de<br />

Sabinas-Lampazos, northwest <strong>of</strong> Sabinas Hidalgo, Nuevo<br />

Leon.<br />

The Lower Albian zone <strong>of</strong> Hypacanthoplites bakeri Scott

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